UCL Discovery
UCL home » Library Services » Electronic resources » UCL Discovery

The First Swift Intensive AGN Accretion Disk Reverberation Mapping Survey

Edelson, R; Gelbord, J; Cackett, E; Peterson, BM; Horne, K; Barth, AJ; Starkey, DA; ... Villforth, C; + view all (2019) The First Swift Intensive AGN Accretion Disk Reverberation Mapping Survey. Astrophysical Journal , 870 (2) , Article 123. 10.3847/1538-4357/aaf3b4. Green open access

[thumbnail of BreeveldEdelson_2019_ApJ_870_123.pdf]
Preview
Text
BreeveldEdelson_2019_ApJ_870_123.pdf - Published Version

Download (4MB) | Preview

Abstract

Swift intensive accretion disk reverberation mapping of four AGN yielded light curves sampled ∼200–350 times in 0.3–10 keV X-ray and six UV/optical bands. Uniform reduction and cross-correlation analysis of these data sets yields three main results: (1) The X-ray/UV correlations are much weaker than those within the UV/optical, posing severe problems for the lamp-post reprocessing model in which variations in a central X-ray corona drive and power those in the surrounding accretion disk. (2) The UV/optical interband lags are generally consistent with t l µ 4 3 as predicted by the centrally illuminated thin accretion disk model. While the average interband lags are somewhat larger than predicted, these results alone are not inconsistent with the thin disk model given the large systematic uncertainties involved. (3) The one exception is the U band lags, which are on average a factor of ∼2.2 larger than predicted from the surrounding band data and fits. This excess appears to be due to diffuse continuum emission from the broad-line region (BLR). The precise mixing of disk and BLR components cannot be determined from these data alone. The lags in different AGN appear to scale with mass or luminosity. We also find that there are systematic differences between the uncertainties derived by JAVELIN versus more standard lag measurement techniques, with JAVELIN reporting smaller uncertainties by a factor of 2.5 on average. In order to be conservative only standard techniques were used in the analyses reported herein

Type: Article
Title: The First Swift Intensive AGN Accretion Disk Reverberation Mapping Survey
Open access status: An open access version is available from UCL Discovery
DOI: 10.3847/1538-4357/aaf3b4
Publisher version: https://doi.org/10.3847/1538-4357/aaf3b4
Language: English
Additional information: This version is the version of record. For information on re-use, please refer to the publisher’s terms and conditions.
Keywords: galaxies: active – galaxies: nuclei – galaxies: Seyfert
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
URI: https://discovery.ucl.ac.uk/id/eprint/10069256
Downloads since deposit
68Downloads
Download activity - last month
Download activity - last 12 months
Downloads by country - last 12 months

Archive Staff Only

View Item View Item